# Axion Gauge Field Inflation and Gravitational Leptogenesis: A Lower Bound on B Modes from the Matter-Antimatter Asymmetry of the Universe

## TL;DR

This paper proposes an axion gauge field inflation model that predicts a distinctive gravitational wave spectrum and links it to matter-antimatter asymmetry via leptogenesis, setting a lower bound on B modes.

## Contribution

It introduces a novel inflation scenario with a blue-tilted, circularly polarized gravitational wave spectrum connected to leptogenesis and matter-antimatter asymmetry.

## Key findings

- Predicts a lower bound on tensor-to-scalar ratio r ~ 0.03-0.04.
- Shows the gravitational wave spectrum is dominated by one polarization.
- Connects gravitational wave signatures to baryogenesis via leptogenesis.

## Abstract

We present a toy model of an axion gauge field inflation scenario that yields viable density and gravitational wave spectra. The scenario consists of an axionic inflaton in a steep potential that is effectively flattened by a coupling to a collection of non-Abelian gauge fields. The model predicts a blue-tilted gravitational wave spectrum that is dominated by one circular polarization, resulting in unique observational targets for cosmic microwave background and gravitational wave experiments. The handedness of the gravitational wave spectrum is incorporated in a model of leptogenesis through the axial-gravitational anomaly; assuming electroweak sphaeleron processes convert the lepton asymmetry into baryons, we predict an approximate lower bound on the tensor-to-scalar ratio r ~ 3-4e-2 for models that also explain the matter-antimatter asymmetry of the Universe.